Table A.3.
Properties of the ASCA sample.
| Name | z | log LX | log LBOL | log LO |
|---|---|---|---|---|
| (1) | (2) | (3) | (4) | (5) |
| Type 2 sources | ||||
| J235554+2836 | 0.729 | 44.87 | 46.36 | – |
| J130453+3548 | 0.316 | 43.91 | 44.79 | – |
| J090053+3856 | 0.229 | 43.94 | 44.54 | – |
| J234725+0053 | 0.213 | 43.93 | 45.19 | – |
| J111432+4055 | 0.153 | 43.77 | 44.25 | – |
| J150339+1016 | 0.095 | 43.26 | 43.80 | – |
| Type 1 sources | ||||
| J001913+1556 | 2.270 | 45.71 | 46.76 | 46.54 |
| J015840+0347 | 0.658 | 44.75 | 46.35 | 45.36 |
| J125732+3543 | 0.524 | 44.56 | 45.69 | 45.21 |
| J002619+1050 | 0.474 | 44.24 | 45.50 | 45.02 |
| J023520−0347 | 0.376 | 44.23 | 45.65 | 44.89 |
| J151441+3650 | 0.371 | 44.83 | 45.96 | 45.30 |
| J144055+5204 | 0.320 | 44.19 | 45.43 | 44.89 |
| J000927−0438 | 0.314 | 43.95 | 44.78 | 44.34 |
| J121427+2936 | 0.309 | 44.25 | 45.03 | 44.90 |
| J122017+0641 | 0.287 | 44.33 | 45.27 | 44.79 |
| J142353+2247 | 0.282 | 44.25 | 45.12 | 44.44 |
| J172938+5230 | 0.278 | 44.13 | 45.41 | 44.98 |
| J103934+5330 | 0.229 | 43.62 | 44.61 | 44.12 |
| J233253+1513 | 0.215 | 44.13 | 44.98 | 44.54 |
| J121854+2957 | 0.178 | 43.64 | 45.16 | 43.63 |
| J170305+4526 | 0.171 | 43.68 | 44.97 | 44.50 |
| J140528+2224 | 0.156 | 43.44 | 44.52 | 44.11 |
| J121359+1404 | 0.154 | 43.26 | 44.36 | 43.92 |
| J170548+2412 | 0.114 | 43.26 | 44.60 | 43.90 |
| J134450+0005 | 0.087 | 42.95 | 44.25 | 43.91 |
| J121930+0643 | 0.081 | 43.00 | 44.52 | 44.14 |
| J144109+3520 | 0.077 | 42.64 | 43.95 | 43.66 |
Notes. Source name; (2) redshift; (3) intrinsic logarithmic hard X-ray luminosity (2–10 keV) in erg s−1 units from Liu et al. (2016) rescaled for our adopted cosmology; (4) SED-fitting derived logarithmic bolometric luminosity in erg s−1 units; (5) B-band 4400 Å AGN logarithmic luminosity in erg s−1 units from the photometric data, provided only for type I sources, because the contamination from the galaxy is negligible.
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